A selected record and an original worked study

1957

Neutron Capture: Competing Clocks

Compare two invented exponential clocks, derive the chance of the first event, and test why slowing both clocks need not change that chance.

Two invented competing clocks, their branching fractions and a common-rate scaling comparison.
0.9
Invented case A: capture first
1/11
Invented case B: capture first
0.1 s
Invented case A: mean wait

The short answer

A process can be slow compared with one rival and fast compared with another. This study turns that relational idea into a small probability model whose assumptions remain visible.

Record comparison

Chance and duration are different quantities

Keep the historical record distinct from the stipulated model.

All numerical fixtures below are invented unless explicitly labelled historical.
QuestionRecord or stipulated inputConsequence and limit
Common scalingMultiply both rates by the same positive factorBranch probability stays fixed; mean wait changes inversely.
A deadlineRun the clocks only until TSome histories have no event before the deadline.

Chronology

A timeline of the turning points

  1. Joint synthesis

    The selected stellar synthesis was published.

The selected stellar argument

BยฒFHโ€™s selected timescale discussion makes neutron capture compete with beta decay at a branching nucleus. Capture times depend on neutron density and cross sections; the authors distinguish nuclei that decay before another capture from those effectively stable during the process.

This is a comparison of mechanisms, not a rule assigning every event to one fixed number of seconds. A branch probability can illuminate the distinction, while remaining much smaller than the paperโ€™s network of reactions.

Sources for this section: [1]

Two stipulated clocks

Invent independent waiting times for capture and decay. Let c and b be constant event rates, measured in sโปยน. In this model the chance of neither event by time t is exp(โˆ’(c+b)t). The density for capture to be first at t is c exp(โˆ’(c+b)t). Integrating from zero to infinity gives P(capture first)=c/(c+b).

The expected wait for either event is 1/(c+b) seconds. These formulas are derived from the stipulated constant-rate exponential clocks; they are not extracted nuclear-rate measurements. A finite exposure, changing environment or additional channel would change the problem.

Sources for this section: [1]

Worked comparison

Case A uses c=9 sโปยน and b=1 sโปยน. Case B uses c=0.1 sโปยน and b=1 sโปยน. Calculate capture-first probability and the mean wait for either event. Then divide both rates in case A by ten. Which answer changes?

Reference answer: A gives 9/10=0.9 and 0.1 s. B gives 1/11โ‰ˆ0.0909 and 10/11โ‰ˆ0.909 s. The scaled A gives 0.9 again, but a mean wait of 1 s. Relative rates determine the branching chance here; their common scale determines the waiting time.

Sources for this section: [1]

What the small model leaves out

The result depends on allowing the clocks to run until one fires. With a deadline T, the unconditional probability that capture occurs first before the deadline becomes c/(c+b)ร—[1โˆ’exp(โˆ’(c+b)T)]. The remaining probability includes histories in which neither event happens.

Thus equal branching fractions need not mean equal outcomes during a short observation window. The exercise explains a distinction in reasoning; it does not reconstruct a star, endorse all historical site assignments or provide nuclear-operating instructions.

Sources for this section: [1]

Continue the chronology

Biography context

Explore United States through connected lives

Connected biographies

The working life behind the record

Quick answers

Common questions

Is a lower event rate automatically the slow process in every context?
No. The model compares it with a specified competing rate; it does not establish a universal threshold.
Are the exercise rates stellar measurements?
No. All rates are invented constant-rate inputs.

Primary and institutional sources

How this history was checked

Selected records support the historical discussion. Invented inputs and original answers are labelled; no complete uninspected work is claimed. This article was reviewed on 31 October 2026.

  1. E. Margaret Burbidge, G. R. Burbidge, William A. Fowler and F. Hoyle, Reviews of Modern Physics 29, 547โ€“650, 1957Synthesis of the Elements in Stars